HR 9038

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HR 9038 A/B/C
Observation data
Epoch 2000      Equinox 2000
Constellation Cepheus
Right ascension 23h 52m 25.31799s[1]
Declination +75° 32′ 40.5141″[1]
Apparent magnitude (V) 6.40[2]/11.4[3]
Characteristics
Spectral type K3 V[4] + M2
U−B color index 0.70[2]
B−V color index 0.98[2]
R−I color index 0.5
Astrometry
Radial velocity (Rv) +4.60[5] km/s
Proper motion (μ) RA: 341.01[1] mas/yr
Dec.: 41.50[1] mas/yr
Parallax (π) 91.82 ± 0.30[1] mas
Distance 35.5 ± 0.1 ly
(10.89 ± 0.04 pc)
Orbit[3]
Primary HR 9038 A
Period (P) 290 yr
Semi-major axis (a) 4.14"
Eccentricity (e) 0.55
Details
HR 9038 A
Surface gravity (log g) 4.71 ± 0.04[6] cgs
Temperature 4,660 ± 110[6] K
Metallicity [Fe/H] 6.62[6] dex
Other designations
BD+74 1047, GJ 909, WDS J23524+7533
HR 9038 A: HD 223778, HIP 117712, HR 9038, SAO 10879

HR 9038 is a ternary star system located thirty-five light-years away, in the constellation Cepheus. Component A is a spectroscopic binary system with an orbital period of 7.753 days and a combined stellar classification of K3 K.[7] Component B component is a red dwarf star that orbits the primary pair every 290 years.[3]

References

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External links


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